The JWST UNCOVER Treasury Survey: Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization

Abstract In this paper we describe the survey design for the Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization (UNCOVER) Cycle 1 JWST Treasury program, which executed its early imaging component in 2022 November. The UNCOVER survey includes ultradeep (∼29–30AB) imaging of ∼45 arcmin 2 on and around the well-studied A2744 galaxy cluster at z = 0.308 and will follow up ∼500 galaxies with extremely deep low-resolution spectroscopy with the NIRSpec/PRISM during the summer of 2023, with repeat visits in summer 2024. We describe the science goals, survey design, target selection, and planned data releases. We also present and characterize the depths of the first NIRCam imaging mosaic, highlighting previously unparalleled resolved and ultradeep 2–4 μ m imaging of known objects in the field. The UNCOVER primary NIRCam mosaic spans 28.8 arcmin 2 in seven filters (F115W, F150W, F200W, F277W, F356W, F410M, and F444W) and 16.8 arcmin 2 in our NIRISS parallel (F115W, F150W, F200W, F356W, and F444W). To maximize early community use of the Treasury data set, we publicly release the full reduced mosaics of public JWST imaging including 45 arcmin 2 NIRCam and 17 arcmin 2 NIRISS mosaics on and around the A2744 cluster, including the Hubble Frontier Field primary and parallel footprints.

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Publication Details

Journal
The Astrophysical Journal
Published
2024-10-01
DOI
https://doi.org/10.3847/1538-4357/ad66cf
Citations
105
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
34.81

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article

The JWST UNCOVER Treasury Survey: Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization

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105 citations
The Astrophysical Journal
Galaxies: Formation, Evolution, Phenomena
34.81
article

The JWST UNCOVER Treasury Survey: Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization

Pratika Dayal, Seiji Fujimoto, Mariska Kriek, Edward N. Taylor, Marla Geha, Camilla Pacifici, Marijn Franx, S. Juneau, Lukas J. Furtak, Rachel Bezanson, Danilo Marchesini, Gourav Khullar, Karl Glazebrook, Sam E. Cutler, Richard Pan, Jenny E. Greene, Ivo Labbé, Adam Muzzin, Casey Papovich, Mauro Stefanon, Themiya Nanayakkara, Susan A. Kassin, Dan Coe, John R. Weaver, David J. Setton, Christina C. Williams, Robert Feldmann, Joel Leja, Pieter van Dokkum, Hakim Atek, Erica J. Nelson, Pascal A. Oesch, Alice E. Shapley, Lamiya Mowla, Gabriel Brammer, Michael V. Maseda, Katherine E. Whitaker, Adi Zitrin, Renske Smit, Sedona H. Price, Anna de Graaff, N. M. Förster Schreiber, Bingjie Wang
article en
105 citations

Abstract

Abstract In this paper we describe the survey design for the Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization (UNCOVER) Cycle 1 JWST Treasury program, which executed its early imaging component in 2022 November. The UNCOVER survey includes ultradeep (∼29–30AB) imaging of ∼45 arcmin 2 on and around the well-studied A2744 galaxy cluster at z = 0.308 and will follow up ∼500 galaxies with extremely deep low-resolution spectroscopy with the NIRSpec/PRISM during the summer of 2023, with repeat visits in summer 2024. We describe the science goals, survey design, target selection, and planned data releases. We also present and characterize the depths of the first NIRCam imaging mosaic, highlighting previously unparalleled resolved and ultradeep 2–4 μ m imaging of known objects in the field. The UNCOVER primary NIRCam mosaic spans 28.8 arcmin 2 in seven filters (F115W, F150W, F200W, F277W, F356W, F410M, and F444W) and 16.8 arcmin 2 in our NIRISS parallel (F115W, F150W, F200W, F356W, and F444W). To maximize early community use of the Treasury data set, we publicly release the full reduced mosaics of public JWST imaging including 45 arcmin 2 NIRCam and 17 arcmin 2 NIRISS mosaics on and around the A2744 cluster, including the Hubble Frontier Field primary and parallel footprints.

The Astrophysical JournalVol. 974(1)
Damien Foundation (BD)
Space Telescope Science Institute, Science and Technology Facilities Council
Partnerships for the goals
Openalex Percentile: Top 0%
Galaxies: Formation, Evolution, Phenomena
34.81
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